Abstract
In this work the low density regions of nuclear and neutron star matter are studied. The search for the existence of pasta phases in this region is performed within the context of the quark-meson coupling (QMC) model, which incorporates quark degrees of freedom. Fixed proton fractions are considered, as well as nuclear matter in beta equilibrium at zero temperature. We analyze the influence of the nuclear pasta on some neutron star properties.
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CITATION STYLE
Grams, G., Santos, A. M., Panda, P. K., Providência, C., & Menezes, D. P. (2020). Pasta Phases Within the QMC Model. In Springer Proceedings in Physics (Vol. 238, pp. 649–652). Springer. https://doi.org/10.1007/978-3-030-32357-8_102
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